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Paper Citation Record · LEDGER

On the Formation of Double Neutron Stars in the Milky Way: Influence of Key Parameters

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2402.04658.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2402.04658 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T11:30:19.874456Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

0
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 21d97593-3ecd-4168-890a-216390790e10 · inbound

Spin evolution and mass distribution of the Galactic Binary Neutron Stars cites this paper.

Spin evolution and mass distribution of the Galactic Binary Neutron Stars On the Formation of Double Neutron Stars in the Milky Way: Influence of Key Parameters

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-11T11:30:19.874456Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T11:30:19.874456Z digest=sha256:d032848b28748ed4474a65b5a121a031996766dde7a9b000a509de1ff15b9061

Observation e6b6a615-3aec-4834-bac0-e8883ed6bdc0 · inbound

Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems cites this paper.

Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems On the Formation of Double Neutron Stars in the Milky Way: Influence of Key Parameters

Reference 44

Resolution
metadata mismatch
local_arxiv, observed 2026-08-06T10:28:55.492682Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-08-06T10:25:57.132031Z digest=sha256:e39a46eb05835d28f7c84bda476256ba20499f382c0198f36e11d236458f5443